遗传算法在含连续/离散变量结构优化中的应用

传统的优化方法难于有效地处理含有连续／离散混合变量优化问题。本文探讨了如何将遗传算法应用于含连续／离散设计变量的结构优化问题。着重讨论了连续／离散混合变量的编码方法和减少适应度函数计算次数的ｍ ｉｃｒｏ ＧＡ 技术。将遗传算法应用于数学考题和十杆结构尺寸／材料混合变量优化问题。两个算例表明,遗传算法能比较有效地解决含连续／离散混合设计变量的优化问题。     

YZL16操纵减摆器仿真研究

ＹＺＬ１６是Ｋ８飞机化操纵减摆器,其操纵和减摆阻尼的液路相互耦合,给设计带来了新的课题。文中采用数字仿真方法研究了ＹＺＬ１６静态阻尼与操纵状态两种工况下的工作特点。仿真中考虑了油液的压缩性,采用阻尼长孔的流量系数计算公式（流量系数是随压差或流量变化的）取代常用的薄壁小孔的固定流量系数。仿真结果与试验结果吻合良好。文中还介绍了阻尼孔直径、阻尼阀的泄漏、控制阀流量特性、油液含气量等各种因素对静态阻尼与     

分析二维导体电磁散射问题的FEM/POPTD方法——TE模(英文)

提出了一种分析计算带有裂缝的二维电大尺寸复杂导体目标电磁散射问题的混合方法—— FEM/ PO-PTD方法。该方法采用基于棱边的有限元法 ( Edge-basedFEM)为低频方法 ,物理光学法与物理绕射理论 ( PO-PTD)为高频方法 ,通过耦合技术将两者结合在一起。本文将该方法应用于带有缝隙的二维导电柱 TE模的电磁散射特性分析 ,计算结果与有关文献的数据一致性很好 ,从而验证了该方法的准确性。文中还给出了另外几种截面的导电柱体雷达截面的计算曲线。理论分析与计算结果表明 ,本文提出的混合方法与其他计算同类问题的方法相比 ,能节省计算机存储单元、提高计算速度     

柱塞泵保持架滑靴安装孔的设计及尺寸计算

在对柱塞泵运动深入分析的基础上,运用坐标变换法和轨迹投影法,使用MATLAB软件,提出了保持架滑靴安装孔尺寸的形成原因及设计计算方法.该方法的优点是:所有的计算公式都为完整的理论计算公式,没有量的取舍;所有的计算结果都为实解,保证了所得的计算结果为真实的理论值.而且一次计算可以得到滑靴安装孔尺寸设计的所有数据.仿真结果表明:设计方法和尺寸计算是正确的.      

航空发动机加速和减速过程最优控制研究

深入研究了航空发动机加速过程和减速过程的最优控制问题。提出了基于改进FSQP(Feasible Sequen-tial Quadratic Programming)算法的航空发动机加速过程和减速过程最优控制方法,仿真结果证明该方法可以在满足航空发动机加速过程和减速过程中各项约束条件的前提下,实现最优的控制目标。     

静叶栅上游端壁双射流气膜冷却特性实验

为了进一步挖掘上游端壁气膜冷却的潜力,在低速叶栅风洞的静叶片上游端壁上,实验研究了双射流构型的气膜冷却特性,并与双排圆孔进行了对比。探究了吹风比(M=0.5,1.0,1.5,2.0)、密度比(Rd=1.0,1.5)的效应。端壁表面的气膜冷却效率通过压力敏感漆(PSP)测得。结果表明,吹风比的增大虽然会加剧吹离现象,但同时也会促进叶栅通道中、后段的气膜覆盖。密度比的增大会抑制气膜吹离,促进气膜横向覆盖和提高平均冷却效率。双射流孔相比于圆形孔,冷却气流在孔下游形成了反肾形涡,较好抑制了气膜吹离;但从双射流孔喷出的冷却气流对于叶栅通道内的涡系也更加敏感。在高吹风比下,双射流孔的冷却效率相对于圆形孔有一定的优势,特别是双射流I构型。     

镜像生物分子

生物分子的手性均一性是地球上生命的重要标志.生命对D型核糖和L型氨基酸的依赖究竟是生命起源的必然,还是早期地球上发生的一次偶然事件,目前尚无定论.地球上生命手性均一性的原因还未能被很好地解释,但一些实验证据已显示基于L型核糖和D型氨基酸的镜像生命被合成出来的可能性.本文简要总结了当前对镜像生物分子的研究进展和方向,并探...     

LaSr3Fe3O10-δ混合导体结构及氧非化学计量的研究

采用柠檬酸盐法制备了纯的LaSr3Fe3O10-δ粉体。利用间接碘量法测定了LaSr3Fe3O10-δ系列样品中铁离子的平均价态和氧的非化学计量值。实验发现,随着温度的逐渐升高,LaSr3Fe3O10-δ逐渐失氧,三价铁浓度增加使得铁的平均价态降低。     

Experimental study on rotary ultrasonic vibration assisted drilling rock

Traditional rotary ultrasonic vibration drilling rock (f_z < 2A) is an effective drilling rock method, but its feed rate is limited by the ultrasonic vibration amplitude, resulting in lower drilling efficiency. In this paper, based on the requirements of drilling efficiency in the asteroid sampling mission, the process method of rotary ultrasonic vibration assisted drilling rock (f_z > 2A) was proposed. The mechanism of ultrasonic vibration assisted drilling rock was analyzed, and the propagation of ultrasonic energy in the process of ultrasonic vibration assisted drilling rock was analyzed. Using the small diameter cemented carbide triangular bit as the drilling tool, the comparative test of ultrasonic vibration assisted drilling and traditional drilling of sandstone, marble, and basalt was carried out. The experimental results showed that there was a specific feed rate range for each type of rock, so that the weight on bit required for ultrasonic vibration assisted drilling was less than that of traditional drilling. With the increase of firmness coefficient of sandstone, marble, and basalt, the ratio of weight on bit to feed rate was increased, and the effective feed rate range of ultrasonic vibration assisted drilling was reduced. The ultrasonic vibration assisted drilling rock (f_z > 2A) was one of the alternative methods for drilling rock on the asteroid surface.     

Pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method

In order to shorten the data update period and further improve the accuracy, a pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method is proposed. The asynchronous overlapping observation method partially overlaps the two adjacent observation periods, so that the data update period depends on the minimum pulsar observation period rather than the maximum like the other algorithms. The number of sampling points is also reduced to 2, which will effectively reduce the calculation burden. The proposed pre-correction extended Kalman filter uses observation data of adjacent sampling points to achieve a two-fold correction and makes up for the problem of insufficient observations on some sampling points caused by the observation method. Finally, simulations show that the proposed algorithm reduces the position and velocity errors by 21.55% and 19.13% compared to the EKF based on asynchronous observation method when using three detectors to observe the corresponding pulsars simultaneously. At the same time, the running time of one data update calculation is only 6.6% more than that of the EKF algorithm based on synchronous observation method.